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| RX J1236.2+2558 , the SIMBAD biblio (12 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST02:09:07 |
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
|
1996A&A...305...74V |
183 | 41 | ROSAT observations of three edge-on spiral galaxies. | VOGLER A., PIETSCH W. and KAHABKA P. | |||||
| 2002A&A...392..817F | 40 | 59 | XMM-Newton observations of ultraluminous X-ray sources in nearby galaxies. | FOSCHINI L., DI COCCO G., HO L.C., et al. | |||||
| 2002ApJ...576..738W | 1 | 14 | 43 | The nature of ultraluminous X-ray sources in NGC 4565. | WU H., XUE S.-J., XIA X.Y., et al. | ||||
|
2002ApJS..143...25C |
155 | 187 | A catalog of candidate intermediate-luminosity X-ray objects. | COLBERT E.J.M. and PTAK A.F. | |||||
| 2003ApJ...583..145T | 1 | 59 | 299 | Chandra snapshot observations of low-luminosity active galactic nuclei with a compact radio source. | TERASHIMA Y. and WILSON A.S. | ||||
| 2003ApJ...595..727I | 99 | 14 | A deep Chandra X-ray observation of NGC 1637. | IMMLER S., WANG Q.D., LEONARD D.C., et al. | |||||
|
2004ApJ...601..735T |
144 | 64 | The luminous X-ray source population in M51 observed with Chandra. | TERASHIMA Y. and WILSON A.S. | |||||
|
2005A&A...429.1125L |
339 | 66 | A catalogue of ultraluminous X-ray sources in external galaxies. | LIU Q.Z. and MIRABEL I.F. | |||||
|
2005ApJS..157...59L |
840 | 130 | Ultraluminous X-ray sources in nearby galaxies from ROSAT high resolution imager observations I. Data analysis. | LIU J.-F. and BREGMAN J.N. | |||||
| 2006A&A...454...77L | 158 | 15 | Toward a clean sample of ultra-luminous X-ray sources. | LOPEZ-CORREDOIRA M. and GUTIERREZ C.M. | |||||
| 2007A&A...472...87G | 37 | X | 1 | 15 | 5 | Eight more ultra luminous X-ray candidates unmasked. | GUTIERREZ C.M. and LOPEZ-CORREDOIRA M. | ||
|
2008ApJ...687..471B |
15 | D | 2 | 117 | 49 | Testing the paradigm that ultraluminous X-ray sources as a class represent accreting intermediate-mass black holes. | BERGHEA C.T., WEAVER K.A., COLBERT E.J.M., et al. |